{"title":"斯托克斯参数和磁场矢量的分布","authors":"Ye Shi-hui","doi":"10.1016/0146-6364(80)90033-X","DOIUrl":null,"url":null,"abstract":"<div><p>On the basis of our numerical solution of the equations of transfer of Stokes parameters, we have established in this paper a method for the determination of the magnetic field strength <em>H</em> and the angle between the field line and the line of sight γ, using observed profile of parameter <em>Q</em>.</p></div>","PeriodicalId":100241,"journal":{"name":"Chinese Astronomy","volume":"4 4","pages":"Pages 402-405"},"PeriodicalIF":0.0000,"publicationDate":"1980-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0146-6364(80)90033-X","citationCount":"0","resultStr":"{\"title\":\"The profiles of the stokes parameters and the magnetic field vector\",\"authors\":\"Ye Shi-hui\",\"doi\":\"10.1016/0146-6364(80)90033-X\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>On the basis of our numerical solution of the equations of transfer of Stokes parameters, we have established in this paper a method for the determination of the magnetic field strength <em>H</em> and the angle between the field line and the line of sight γ, using observed profile of parameter <em>Q</em>.</p></div>\",\"PeriodicalId\":100241,\"journal\":{\"name\":\"Chinese Astronomy\",\"volume\":\"4 4\",\"pages\":\"Pages 402-405\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1980-12-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/0146-6364(80)90033-X\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Chinese Astronomy\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/014663648090033X\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Astronomy","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/014663648090033X","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The profiles of the stokes parameters and the magnetic field vector
On the basis of our numerical solution of the equations of transfer of Stokes parameters, we have established in this paper a method for the determination of the magnetic field strength H and the angle between the field line and the line of sight γ, using observed profile of parameter Q.